Were recently reported MHz events planet mass primordial black hole mergers?
Abstract A bulk acoustic wave cavity as high frequency gravitational wave antenna has recently detected two rare events at 5.5MHz. Assuming that the detected events are due to gravitational waves, their characteristic strain amplitude lies at about $$h_c\approx 2.5 \times 10^{-16}$$ h c ≈ 2.5 × 10 -...
Guardado en:
Autor principal: | |
---|---|
Formato: | article |
Lenguaje: | EN |
Publicado: |
SpringerOpen
2021
|
Materias: | |
Acceso en línea: | https://doaj.org/article/a302e84b0b8441d49509328b981ed162 |
Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
id |
oai:doaj.org-article:a302e84b0b8441d49509328b981ed162 |
---|---|
record_format |
dspace |
spelling |
oai:doaj.org-article:a302e84b0b8441d49509328b981ed1622021-11-28T12:11:49ZWere recently reported MHz events planet mass primordial black hole mergers?10.1140/epjc/s10052-021-09853-81434-60441434-6052https://doaj.org/article/a302e84b0b8441d49509328b981ed1622021-11-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09853-8https://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract A bulk acoustic wave cavity as high frequency gravitational wave antenna has recently detected two rare events at 5.5MHz. Assuming that the detected events are due to gravitational waves, their characteristic strain amplitude lies at about $$h_c\approx 2.5 \times 10^{-16}$$ h c ≈ 2.5 × 10 - 16 . While a cosmological signal is out of the picture due to the large energy carried by the high frequency waves, the signal could be due to the merging of two planet mass primordial black holes ( $$\approx 4\times 10^{-4} M_\odot $$ ≈ 4 × 10 - 4 M ⊙ ) inside the Oort cloud at roughly 0.025 pc (5300 AU) away. In this short note, we show that the probability of one such event to occur within this volume per year is around $$1:10^{24}$$ 1 : 10 24 , if such Saturn-like mass primordial black holes are $$1\%$$ 1 % of the dark matter. Thus, the detected signal is very unlikely to be due the merger of planet mass primordial black holes. Nevertheless, the stochastic background of saturn mass primordial black holes binaries might be seen by next generation gravitational wave detectors, such as DECIGO and BBO.Guillem DomènechSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 11, Pp 1-6 (2021) |
institution |
DOAJ |
collection |
DOAJ |
language |
EN |
topic |
Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
spellingShingle |
Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Guillem Domènech Were recently reported MHz events planet mass primordial black hole mergers? |
description |
Abstract A bulk acoustic wave cavity as high frequency gravitational wave antenna has recently detected two rare events at 5.5MHz. Assuming that the detected events are due to gravitational waves, their characteristic strain amplitude lies at about $$h_c\approx 2.5 \times 10^{-16}$$ h c ≈ 2.5 × 10 - 16 . While a cosmological signal is out of the picture due to the large energy carried by the high frequency waves, the signal could be due to the merging of two planet mass primordial black holes ( $$\approx 4\times 10^{-4} M_\odot $$ ≈ 4 × 10 - 4 M ⊙ ) inside the Oort cloud at roughly 0.025 pc (5300 AU) away. In this short note, we show that the probability of one such event to occur within this volume per year is around $$1:10^{24}$$ 1 : 10 24 , if such Saturn-like mass primordial black holes are $$1\%$$ 1 % of the dark matter. Thus, the detected signal is very unlikely to be due the merger of planet mass primordial black holes. Nevertheless, the stochastic background of saturn mass primordial black holes binaries might be seen by next generation gravitational wave detectors, such as DECIGO and BBO. |
format |
article |
author |
Guillem Domènech |
author_facet |
Guillem Domènech |
author_sort |
Guillem Domènech |
title |
Were recently reported MHz events planet mass primordial black hole mergers? |
title_short |
Were recently reported MHz events planet mass primordial black hole mergers? |
title_full |
Were recently reported MHz events planet mass primordial black hole mergers? |
title_fullStr |
Were recently reported MHz events planet mass primordial black hole mergers? |
title_full_unstemmed |
Were recently reported MHz events planet mass primordial black hole mergers? |
title_sort |
were recently reported mhz events planet mass primordial black hole mergers? |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/a302e84b0b8441d49509328b981ed162 |
work_keys_str_mv |
AT guillemdomenech wererecentlyreportedmhzeventsplanetmassprimordialblackholemergers |
_version_ |
1718408158378983424 |